弹体孔缝耦合特性研究

针对弹体上孔缝在微波脉冲作用下的耦合特性,利用电磁仿真软件CST进行分析,并研究不同孔缝形状、大小以及分布方式对耦合强度和共振频率的影响。研究结果表明,对于单个孔缝,正方形和圆形孔缝的耦合系数较为接近,且随着频率增高而增大;当入射电磁波电场方向与矩形孔缝的长边垂直时,耦合系数最大,此时将发生共振,共振频率对应的二分之一波长约等于矩形孔缝的长边长度;当入射电磁波电场方向与矩形孔缝的长边平行时,耦合系数最小。文中还进一步研究耦合系数与矩形长宽比例的关系。最后,研究组成孔缝阵列时的情况,发现各种形状的孔缝耦合系数均有明显下降,且孔缝形状差异的影响不再明显。     

基于SPT70的微波霍尔推力器谐振腔电磁特征计算分析

微波霍尔推力器是双极霍尔推力器的一种形式,其电离源中的圆柱谐振腔是一个关键件,它承担着微波能量的传输并激发表面波等离子体的重要作用。正确选择其结构和谐振模态是构建微波霍尔推力器的重要基础。为此,针对不同结构、不同谐振模态的微波谐振腔进行结构参数计算分析和电磁场分布规律数值模拟,从中选取可以和霍尔推力器SPT70加速通道相匹配的腔体结构。计算分析和数值模拟结果表明2.45GHz谐振于TM011模的圆柱谐振腔和SPT70加速通道有合适的匹配关系。     

TC4 钛合金板材双晶探头超声波检测

研究了TC4钛合金板材高灵敏度双晶探头超声波检测中变型波、组织噪声的产生原因及影响.结果表明:变型波会给缺陷波定量评定带来影响,以缺陷波始脉冲波幅定量评定最为准确,对于缺陷波始脉冲之后的波幅超标应选用不同焦距的双晶探头进行对比检测.组织噪声的产生与板材中同取向粗大α相晶粒增多密切相关,通过减小脉冲宽度可有效降低组织噪声.     

偏置功率匹配器在微波小功率校准系统8mm频段应用

为了提高8mm微波小功率敏感器的校准准确度,利用原有的SYSTEMⅡ微波小功率标准系统,通过研制偏置功率匹配器,在8mm频段构建了新型波导小功率敏感器校准系统。本文详细叙述了偏置功率匹配器的设计及其工作原理,该系统具有操作方便、性能稳定等优点,可实现对8mm波导小功率敏感器的准确校准。     

OMEGA型空间太阳能电站聚光系统设计

空间太阳能电站聚光系统的尺度在千米级,聚光系统的方案设计涉及光、机、电、热及控制等多个学科。现有的空间太阳能电站聚光系统的设计方案不同程度上存在太阳光收集效率低、收集功率波动大、聚光系统质量高、控制系统复杂等不足。因此,需要综合考虑各种因素,提出高效、稳定、轻质和控制简单的聚光系统设计方案。文章对SSPS-ALPHA方案的聚光系统作了深入分析,并基于与 ALPHA方案相同的能量传输假设,针对ALPHA方案的不足提出了一种新的聚光系统设计方案,称之为 SSPS-OMEGA方案。通过比对分析,在与ALPHA聚光方案相同收集功率的前提下,OMEGA聚光方案不仅可以高效、稳定地收集太阳光,而且 OMEGA方案的功率质量比比ALPHA方案提升了31.68％。     

Spin parameters of High Earth Orbiting satellites Etalon-1 and Etalon-2 determined from kHz Satellite Laser Ranging data

The high repetition rate Satellite Laser Ranging (SLR) system developed in Graz, Austria, measures ranges to the High Earth Orbiting satellites Etalon-1 and Etalon-2 with the millimeter accuracy. The 2 kHz repetition rate of the laser and the relatively high return rates allow to use the SLR data to calculate the spin parameters of the Etalon satellites. The analysis of the 10 years (October 2003–September 2013) of the SLR data gives trends of the spin axes orientation (J2000 Inertial Reference Frame):     

Microwave Brightness Temperature and Lunar Soil Dielectric Property Retrieve

Among many scientific objectives of lunar exploration, investigations on lunar soil become more and more attractive to the scientists duo to the existence of abundant 3He and ilmenite in the lunar soil and their possible utilization. Although the soil composition determination on the lunar surface is available by visible light spectrometer,γ/X-ray spectrometer etc, the evaluations on the total reserves of 3He and ilmenite in the lunar deep and on the thickness of the lunar soil are still impossible so far. In this paper, the authors first give a rough analysis of the microwave brightness temperature images of the lunar disc observed using the NRAO 12 Meter Telescope and Siberian Solar Radio Telescope; then introduce our researches on the microwave dielectric properties of lunar soil simulators; finally, discuss some basic relations between the microwave brightness temperature and lunar soil properties.     

Measured properties of the cosmic background radiation

After a pioneering period when the observers were mainly interested in checking the general properties of the Cosmic Background Radiation through observations at still higher frequencies, the observational efforts are now devoted to the discovery of features in the mean panorama, in particular :i) Distortions in the frequency spectrum, ii) Spatial anisotropies at various angular scales; iii) Polarization. The observational information is reviewed.     

Simulations of the microwave sky and of its “observations”

Here follows a preliminary report on the construction of fake millimeter and sub-millimeter skies, as observed by virtual instruments,e.g. the COBRA/SAMBA mission, using theoretical modeling and data extrapolations. Our goal is to create maps as realistic as possible of the relavant physical contributions which may contribute to the detected signals. This astrophysical modeling is followed by simulations of the measurement process itself by a given instrumental configuration. This will enable a precise determination of what can and cannot be achieved with a particular experimental configuration, and provide a feedback on how to improve the overall design. It is a key step on the way to define procedures for the separation of the different physical processes in the future observed maps. Note that this tool will also prove useful in preparing and analyzing current (e.g. balloon borne) Microwave Background experiments.     

Spin motion determination of the Envisat satellite through laser ranging measurements from a single pass measured by a single station

The Satellite Laser Ranging (SLR) technology is used to accurately determine the position of space objects equipped with so-called retro-reflectors or retro-reflector arrays (RRA). This type of measurement allows to measure the range to the spacecraft with high precision, which leads to determination of very accurate orbits for these targets. Non-active spacecraft, which are not attitude controlled any longer, tend to start to spin or tumble under influence of the external and internal torques and forces.If the return signal is measured for a non-spherical non-active rotating object, the signal in the range residuals with respect to the reference orbit is more complex. For rotating objects the return signal shows an oscillating pattern or patterns caused by the RRA moving around the satellite’s centre of mass. This behaviour is projected onto the radial component measured by the SLR.In our work, we demonstrate how the SLR ranging technique from one sensor to a satellite equipped with a RRA can be used to precisely determine its spin motion during one passage. Multiple SLR measurements of one target over time allow to accurately monitor spin motion changes which can be further used for attitude predictions. We show our solutions of the spin motion determined for the non-active ESA satellite Envisat obtained from measurements acquired during years 2013–2015 by the Zimmerwald SLR station, Switzerland. All the necessary parameters are defined for our own so-called point-like model which describes the motion of a point in space around the satellite centre of mass.